Results 91 to 100 of about 1,099 (180)

Are WASP-107-like Systems Consistent with High-eccentricity Migration?

open access: yesThe Astrophysical Journal
WASP-107 b seems to be a poster child of the long-suspected high-eccentricity migration scenario. It is on a 5.7 day, polar orbit. The planet is Jupiter-like in radius but Neptune-like in mass with exceptionally low density.
Hang Yu, Fei Dai
doaj   +1 more source

No Strong Associations between Eccentricity and Orbital Architecture in Kepler Compact Multis

open access: yesThe Astronomical Journal
The dynamical history of a planetary system is recorded in the present day architecture of its constituent planets’ sizes, orbital periods, and eccentricities.
Gregory J. Gilbert   +2 more
doaj   +1 more source

Planet Mass Function around M Stars at 1–10 au: A Plethora of Sub-Earth Mass Objects

open access: yesThe Astrophysical Journal
Small planets (≲1 M _⊕ ) at intermediate orbital distances (∼1 au) represent an uncharted territory in exoplanetary science. The upcoming microlensing survey by the Nancy Grace Roman Space Telescope will be sensitive to objects as light as Ganymede and ...
Yayaati Chachan, Eve J. Lee
doaj   +1 more source

Boundary Layers of Circumplanetary Disks around Spinning Planets. II. Global Modes with Azimuthal Magnetic Fields

open access: yesThe Astrophysical Journal
The accretion of material from disks onto weakly magnetized objects invariably involves its traversal through a material surface, known as the boundary layer (BL).
Zhihao Fu, Shunquan Huang, Cong Yu
doaj   +1 more source

Constraints on the Orbit of the Young Substellar Companion GQ Lup B from High-resolution Spectroscopy and VLTI/GRAVITY Astrometry

open access: yesThe Astrophysical Journal
Understanding the orbits of giant planets is critical for testing planet formation models, particularly at wide separations (>10 au) where traditional core accretion becomes inefficient.
Vidya Venkatesan   +101 more
doaj   +1 more source

Magma Ocean Interactions Can Explain JWST Observations of the Sub-Neptune TOI-270 d

open access: yesThe Astrophysical Journal
Sub-Neptunes with substantial atmospheres may possess magma oceans in contact with the overlying gas, with chemical interactions between the atmosphere and magma playing an important role in shaping atmospheric composition.
Matthew C. Nixon   +11 more
doaj   +1 more source

Euhabitability: A New Term to Aid in the Search for Life in Addition to the Habitable Zone Framework. [PDF]

open access: yesSpace Sci Rev
Glaser DM   +7 more
europepmc   +1 more source

Computational challenges in exoplanet atmospheric retrieval. [PDF]

open access: yesLiving Rev Comput Astrophys
K Barstow J, Welbanks L.
europepmc   +1 more source

Lightning initiation on the exoplanet K2-18b. [PDF]

open access: yesSci Rep
Fangel-Lloyd E   +5 more
europepmc   +1 more source

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